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Titel |
Astronomical Theory of Early Human Migration (Milutin Milankovic Medal Lecture) |
VerfasserIn |
Axel Timmermann, Tobias Friedrich |
Konferenz |
EGU General Assembly 2017
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Medientyp |
Artikel
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Sprache |
en
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Digitales Dokument |
PDF |
Erschienen |
In: GRA - Volume 19 (2017) |
Datensatznummer |
250139100
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Publikation (Nr.) |
EGU/EGU2017-2276.pdf |
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Zusammenfassung |
Our climate system varies on a wide range of timescales, from seasons to several millions of
years. A large part of this variability is internally generated as a result of instabilities of the
coupled atmosphere-ocean-ice-carbon cycle system. Other modes of variability,
such as glacial cycles, are caused by astronomical forcings with periods of 20,
40, 100 thousand years. These so-called Milankovitch Cycles are associated with
earth’s axis wobble, axis obliquity and shifts in the eccentricity of earth’s orbit
around the sun, respectively. When these cycles conspire, they can cause the climate
system to plunge into an ice-age. This happened last time 110,000 years ago,
when Northern Hemisphere summer radiation decreased substantially and ice-sheets
started to form as a result. Around 100,000 years ago northern Hemisphere summer
moved again closer to the sun and Homo sapiens started to leave Africa across
vegetated corridors in Northeastern Africa and the Arabian Peninsula. This first
migration wave must have been relatively weak, but it left unequivocal traces in the
fossil and archaeological record. Why Homo sapiens embarked on its grand journey
across our planet during glacial climate conditions has been subject of an intense
debate in various scientific communities. Moreover, the archaeological records of an
early exodus around 100 thousand years ago seem to be at odds with paleo-genetic
evidences, that place the first dispersal out of Africa around 70-60 thousand years
ago.
To elucidate what role climate and environmental conditions played in the dispersal of
Anatomically Modern Humans out of Africa, we have developed and applied one of the first
integrated climate/human migration computer models. The model simulates ice-ages,
abrupt climate change, the “peopling” of our planet and captures the arrival time of
Homo sapiens in the Levant, Arabian Peninsula, Southern China and Australia
in close agreement with paleo climate reconstructions, fossil and archaeological
evidence.
The human dispersal model simulates multiple prominent migration waves of Homo
sapiens across the Arabian Peninsula and the Levant region around 106-94, 89-73, 59-47 and
45-29 thousand years ago. These waves were caused by earth’s axis wobble and its
corresponding changes in climate seasonality and resulting large-scale shifts in
vegetation in tropical/subtropical regions. Such shifts opened up green corridors
between Africa, the Sinai and the Arabian Peninsula, enabling Homo sapiens to leave
Northeastern Africa and migrate into Asia, Europe, Australia and eventually into
the Americas. The model also simulates a complex pattern of human dispersal
out of Africa and back flow into Africa, that challenges the more unidirectional
away-from-Africa perspective that is still very prevalent in anthropology and some genetic
studies.
Paleo-genetic reconstructions indicate that the first exodus out of Africa must have
occurred around 70-60 thousand years ago. In contrast, our computer simulations and
paleo-climate data show that northeastern Africa experienced one of its most severe
long-term droughts during this time. The resulting large desert areas would have been an
impenetrable natural border for early human migration.
More research needs to be done to help reconcile and synthesize genetic, archaeological,
climatological and anthropological data. |
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